Table 4.
Fraction of outliers in the TOA datasets.
Pulsar | 1D F8 | 2D | 1D fscrunch |
---|---|---|---|
J0023+0923 | 53.8% | 5.3% | 3.8% |
J0610−2100 | 9.1% | 2.1% | 1.1% |
J0636+5128 | 12.2% | 3.4% | 1.5% |
J1124−3653 | 82.1% | 60.3% | 56.3% |
J1513−2550 | 18.8% | 5.4% | 6.8% |
J1544+4937 | 34.8% | 2.9% | 2.6% |
J1555−2908 | 13.9% | 6.4% | 6.4% |
J1705−1903 | 0.6% | 0.0% | 0.0% |
J1719−1438 | 68.8% | 2.0% | 1.0% |
J1731−1847 | 41.4% | 28.1% | 77.4% |
J1745+1017 | 16.4% | 1.2% | 2.4% |
J1959+2048 | 43.4% | 6.6% | 8.9% |
J2051−0827 | 9.0% | 3.1% | 3.4% |
J2055+3829 | 17.4% | 11.5% | 11.7% |
J2115+5448 | 36.2% | 23.5% | 40.4% |
J2214+3000 | 90.2% | 5.3% | 4.0% |
J2234+0944 | 14.4% | 6.5% | 6.4% |
J2256−1024 | 48.2% | 5.4% | 5.1% |
Notes. For each pulsars we compared TOAs extracted from eight frequency sub-bands of 64 MHz each using the standard template-matching method (“1D F8”), and TOAs extracted using the entire available bandwidth, with the wideband template-matching technique as implemented in the PulsePortraiture library (“2D”). For reference we also list the outlier rates as obtained when extracting TOAs from fully frequency-scrunched observations (“1D fscrunch”). Outliers are defined here are those with residuals larger than 1% of Pspin considering the uncertainty.
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